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The Differential Redshift of Titanium Lines in K Stars

We present measurements of line core positions in UVES spectra of a sample of K-type stars, using the technique of bisector tracing. In all but two of these stars we detect an excess redshift of Ti I lines with respect to Fe I lines. We explain this invoking the temperature-dependence of the line de...

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Detalles Bibliográficos
Publicado en:Revista Mexicana de Astronomía y Astrofísica
Principais autores: Benjamin Oostra, Paula Catalina Vargas Muñoz
Formato: Artigo
Idioma:Inglês
Publicado: Universidad Nacional Autónoma de México 2022
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Acceso en liña:https://www.redalyc.org/articulo.oa?id=57175502001
https://www.redalyc.org/journal/571/57175502001/
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https://www.redalyc.org/journal/571/57175502001/57175502001.epub
https://www.redalyc.org/journal/571/57175502001/movil
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